1.0KMI - Nagoya Universityhttps://www.kmi.nagoya-u.ac.jp/engHadronic Interactions and Ultra-High Energy Cosmic Rays - KMI - Nagoya Universityrich600338<blockquote class="wp-embedded-content" data-secret="TxKoM9fv3q"><a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/811/">Hadronic Interactions and Ultra-High Energy Cosmic Rays</a></blockquote><iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/811/embed/#?secret=TxKoM9fv3q" width="600" height="338" title="“Hadronic Interactions and Ultra-High Energy Cosmic Rays” — KMI - Nagoya University" data-secret="TxKoM9fv3q" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"></iframe><script type="text/javascript">
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On the one hand, the uncertainty in the prediction of shower observables for different primary particles and energies is currently dominated by differences between hadronic interaction models. Since the end of 2009, LHC data has become available for proton-proton scattering at different energies, extending to the reach of collider data. The LHC data on minimum bias measurements can be used to test Monte Carlo generators and these new constrains will help to reduce the uncertainties in air shower predictions. On …